Fig. 7.
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Quasi-bolometric (UV and optical) light curves for SN 2018xx (magenta circles) and SN 2019gbx (green rhombuses) compared with that of SN 2004eo (orange stars) (Pastorello et al. 2007; Li et al. 2022). The solid red curve and dashed dark green curve represent the Arnett (1982) radiation diffusion model of SN 2018xx and SN 2019gbx, respectively.
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